| dc.contributor.advisor | Koten, Pavel | |
| dc.creator | Vojáček, Vlastimil | |
| dc.date.accessioned | 2017-04-20T15:40:08Z | |
| dc.date.available | 2017-04-20T15:40:08Z | |
| dc.date.issued | 2009 | |
| dc.identifier.uri | http://hdl.handle.net/20.500.11956/27360 | |
| dc.description.abstract | In the present work we study the Orionid 2006 meteor shower. All results in this work come from double station video observations. We study exceptional activity, caused most probably by particles trapped in resonance motion with Jupiter. We focused on light curves, atmospheric trajectories and orbital elements of meteoroids. We can find here comparison with other years of activity of the Orionid meteor shower and comparison with other annual meteor showers. | en_US |
| dc.language | Čeština | cs_CZ |
| dc.language.iso | cs_CZ | |
| dc.publisher | Univerzita Karlova, Matematicko-fyzikální fakulta | cs_CZ |
| dc.title | Vlastnosti Orionid pozorovaných v roce 2006 | cs_CZ |
| dc.type | diplomová práce | cs_CZ |
| dcterms.created | 2009 | |
| dcterms.dateAccepted | 2009-09-15 | |
| dc.description.department | Astronomical Institute of Charles University | en_US |
| dc.description.department | Astronomický ústav UK | cs_CZ |
| dc.description.faculty | Faculty of Mathematics and Physics | en_US |
| dc.description.faculty | Matematicko-fyzikální fakulta | cs_CZ |
| dc.identifier.repId | 61675 | |
| dc.title.translated | Properties of the Orionid meteors observed in 2006 | en_US |
| dc.contributor.referee | Šolc, Martin | |
| dc.identifier.aleph | 001139375 | |
| thesis.degree.name | Mgr. | |
| thesis.degree.level | navazující magisterské | cs_CZ |
| thesis.degree.discipline | Astronomie a astrofyzika | cs_CZ |
| thesis.degree.discipline | Astronomy and Astrophysics | en_US |
| thesis.degree.program | Fyzika | cs_CZ |
| thesis.degree.program | Physics | en_US |
| uk.thesis.type | diplomová práce | cs_CZ |
| uk.taxonomy.organization-cs | Matematicko-fyzikální fakulta::Astronomický ústav UK | cs_CZ |
| uk.taxonomy.organization-en | Faculty of Mathematics and Physics::Astronomical Institute of Charles University | en_US |
| uk.faculty-name.cs | Matematicko-fyzikální fakulta | cs_CZ |
| uk.faculty-name.en | Faculty of Mathematics and Physics | en_US |
| uk.faculty-abbr.cs | MFF | cs_CZ |
| uk.degree-discipline.cs | Astronomie a astrofyzika | cs_CZ |
| uk.degree-discipline.en | Astronomy and Astrophysics | en_US |
| uk.degree-program.cs | Fyzika | cs_CZ |
| uk.degree-program.en | Physics | en_US |
| thesis.grade.cs | Výborně | cs_CZ |
| thesis.grade.en | Excellent | en_US |
| uk.abstract.en | In the present work we study the Orionid 2006 meteor shower. All results in this work come from double station video observations. We study exceptional activity, caused most probably by particles trapped in resonance motion with Jupiter. We focused on light curves, atmospheric trajectories and orbital elements of meteoroids. We can find here comparison with other years of activity of the Orionid meteor shower and comparison with other annual meteor showers. | en_US |
| uk.file-availability | V | |
| uk.publication.place | Praha | cs_CZ |
| uk.grantor | Univerzita Karlova, Matematicko-fyzikální fakulta, Astronomický ústav UK | cs_CZ |
| dc.identifier.lisID | 990011393750106986 | |
